To be able to place EPIC 205375290 in the HR-diagram and learn more about the star's properties, we first analyzed a low resolution (R=3200) optical spectrum obtained with the RSS spectrograph [1]}, [2]} mounted at the South African Large Telescope [3]}. We identify Lii 6708 Å to be in absorption and found emission in the hydrogen Balmer lines and Caii H&K lines. These features are superimposed on a late-type spectrum with prominent TiO absorption bands. Such a spectroscopic pattern is in agreement with the young evolutionary stage of EPIC 205375290. Comparing the depths and shapes of the TiO bandheads with the template spectra from the MILES library [4]}, we confirm the spectral class of EPIC 205375290 to be dM1e, which is in agreement with the previous determination by [5]}.
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